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Journal ArticleDOI

Application of the Information Criterion to the Estimation of Galaxy Luminosity Function

Tsutomu T. Takeuchi
- 01 May 2000 - 
- Vol. 271, Iss: 3, pp 213-226
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TLDR
In this article, the authors applied Akaike's Information Criterion (AIC) to the determination of the shape of the luminosity function (LF) of galaxies, and derived a formula to obtain the optimal bin number.
Abstract
To determine the exact shape of the luminosity function (LF) of galaxies is one of the central problems in galactic astronomy and observational cosmology. The most popular method to estimate the LF is maximum likelihood, which is clearly understood with the concepts of the information theory. In the field of information theory and statistical inference, great advance has been made by the discovery of Akaike's Information Criterion (AIC). It enables us to perform a direct comparison among different types of model swith different numbers of parameters, and provides us a common basis of the model adequacy. In this paper we applied AIC to the determination of the shape of the LF. We first treated the estimation using stepwise LF(Efstathiou, Ellis and Peterson,1988), and derived a formula to obtain the optimal bin number. In addition, we studied the method to compare the goodness-of-fit of the parametric form (Sandage, Tamman and Yahil, 1979) with stepwise LF.

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Citations
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Dynamics of dark energy

TL;DR: In this article, the authors review the observational evidence for the current accelerated expansion of the universe and present a number of dark energy models in addition to the conventional cosmological constant, paying particular attention to scalar field models such as quintessence, K-essence and tachyon.
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Information criteria for astrophysical model selection

TL;DR: The Deviance Information Criterion as mentioned in this paper combines ideas from both heritages; it is readily computed from Monte Carlo posterior samples and, unlike the AIC and BIC, allows for parameter degeneracy.
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How many cosmological parameters

TL;DR: In this article, the Akaike and Bayesian information criteria are applied to the current cosmological data sets to determine the parameter set providing the preferred fit to the data.
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ISM properties in low-metallicity environments. III. The dust spectral energy distributions of II Zw 40, He 2-10 and NGC 1140

TL;DR: In this paper, the authors present new 450 and 850μm SCUBA data and 1.3 mm MAMBO data of the dwarf galaxies II Zw 40, He 2-10 and NGC 1140.
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Imfit: a fast, flexible new program for astronomical image fitting

TL;DR: In this article, the authors describe an open-source astronomical image-fitting program called IMFIT, specialized for galaxies but potentially useful for other sources, which is fast, flexible, and highly extensible.
References
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Journal ArticleDOI

A new look at the statistical model identification

TL;DR: In this article, a new estimate minimum information theoretical criterion estimate (MAICE) is introduced for the purpose of statistical identification, which is free from the ambiguities inherent in the application of conventional hypothesis testing procedure.
Book

Linear statistical inference and its applications

TL;DR: Algebra of Vectors and Matrices, Probability Theory, Tools and Techniques, and Continuous Probability Models.
Journal ArticleDOI

An analytic expression for the luminosity function for galaxies

TL;DR: In this paper, a new analytic approximation for the luminosity function for galaxies is proposed, which shows good agreement with both a luminosity distribution for bright nearby galaxies and a composite luminosity distributions for cluster galaxies.